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20032011
most citedA synthesis model for AGN evolution: supermassive black holes growth and feedback modes

315 citations · 994 across the 14 of their papers we have counts for

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astro-ph200829 cited

Blazing trails: Microquasars as head-tail sources and the seeding of magnetized plasma into the ISM

S. Heinz, H. J. Grimm, R. A. Sunyaev +1

We discuss the dynamics of microquasar jets in the interstellar medium, with specific focus on the effects of the X-ray binaries' space velocity with respect to the local Galactic…

astro-ph2008315 cited

A synthesis model for AGN evolution: supermassive black holes growth and feedback modes

Andrea Merloni, Sebastian Heinz

We present a comprehensive synthesis model for the AGN evolution and the growth of supermassive black holes in the Universe. We solve the continuity equation for SMBH mass function…

astro-ph200830 cited

A deep Chandra observation of Abell 4059: a new face to radio-mode AGN feedback?

Christopher S. Reynolds, Elyse A. Casper, Sebastian Heinz

A deep Chandra observation of the cooling core cluster Abell 4059 (A4059) is presented. Previous studies have found two X-ray cavities in the central regions of A4059 together with…

astro-ph2007229 cited

Measuring the kinetic power of AGN in the radio mode

Andrea Merloni, Sebastian Heinz

(Abridged) We have studied the relationship among nuclear radio and X-ray power, Bondi rate and the kinetic luminosity of sub-Eddington active galactic nuclear (AGN) jets. Besides…

astro-ph200743 cited

Evidence for a parsec scale X-ray jet from the accreting neutron star Circinus X-1

S. Heinz, N. S. Schulz, W. N. Brandt +1

We analyzed the zero-order image of a 50 ks Chandra gratings observation of Circinus X-1, taken in 2005 during the source's low-flux state. Circinus X-1 is an accreting neutron sta…

astro-ph200756 cited

Shock heating by FR I radio sources in galaxy clusters

M. Brueggen, S. Heinz, E. Roediger +2

Feedback by active galactic nuclei (AGN) is frequently invoked to explain the cut-off of the galaxy luminosity function at the bright end and the absence of cooling flows in galaxy…